dc.creatorRomero, Gustavo Esteban
dc.creatorCellone, Sergio Aldo
dc.creatorCombi, Jorge Ariel
dc.date2000
dc.date2019-10-29T12:35:02Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/84260
dc.identifierissn:0004-6256
dc.descriptionWe report the results of a microvariability monitoring campaign on the southern blazar PKS 0537-441. The source was observed in the V and R optical bands throughout six consecutive nights. Strong variations at both bands, with amplitudes of ∼0.3 mag, were observed on timescales of about 2 days. Smaller fluctuations of ∼0.05 mag on a scale of a couple of hours are superposed on the larger outburst. The spectral index was also variable during the observing period, with an average value of α = -1.6 and changes up to ∼27.5%. The spectrum varies in the sense that it becomes harder when the source is brighter, in accordance with predictions of shock-in-jet models. We discuss our results and the possible origin of the variability in this blazar in light of recent higher frequency observations.
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.descriptionInstituto Argentino de Radioastronomía
dc.formatapplication/pdf
dc.format1192-1197
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Astronómicas
dc.subjectBL lacertae objects: individual (PKS 0537-441)
dc.subjectGalaxies: active
dc.subjectGalaxies: photometry
dc.titleTwo-color photometry with high temporal resolution of the extremely variable blazar PKS 0537-441
dc.typeArticulo
dc.typeArticulo


Este ítem pertenece a la siguiente institución